Emilio Romano-Diaz

Dissecting cosmological filaments at high redshifts: emergence of spaghetti-type flow inside DM haloes

#1

(Oct 2, 2023)

Published in:
- Mon.Not.Roy.Astron.Soc. 527 (2023) 4, 11095-11112
•
e-Print:
- 2310.01369 [astro-ph.GA]

DOI

reference search2 citations

Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop

#2

et al.

(Jan 31, 2023)

Published in:
- Publ.Astron.Soc.Pac. 135 (2023) 1044, 021001
•
e-Print:
- 2301.13611 [astro-ph.SR]

DOI

reference search2 citations

Mechanical feedback from stellar winds with an application to galaxy formation at high redshift

#3

(Jan 18, 2022)

Published in:
- Mon.Not.Roy.Astron.Soc. 512 (2022) 3, 4573-4592
•
e-Print:
- 2201.07244 [astro-ph.GA]

pdfDOI

reference search8 citations

Emergence of galactic morphologies at cosmic dawn: input from numerical modelling

#4

(Dec 15, 2021)

Published in:
- Mon.Not.Roy.Astron.Soc. 513 (2022) 1, 693-712
•
e-Print:
- 2112.08396 [astro-ph.GA]

pdfDOI

reference search1 citation

Radial acceleration relation of

\Lambda

CDM satellite galaxies

#5

(Dec 12, 2017)

Published in:
- Phys.Rev.Lett. 120 (2018) 26, 261301
•
e-Print:
- 1712.04448 [astro-ph.GA]

pdfDOI

reference search16 citations

ZOMG - III. The effect of halo assembly on the satellite population

#6

(Jul 4, 2017)

Published in:
- Mon.Not.Roy.Astron.Soc. 473 (2017) 2, 2234-2250
•
e-Print:
- 1707.01108 [astro-ph.GA]

pdfDOI

reference search17 citations

ZOMG – II. Does the halo assembly history influence central galaxies and gas accretion?

#7

(Jan 10, 2017)

Published in:
- Mon.Not.Roy.Astron.Soc. 469 (2017) 2, 1809-1823
•
e-Print:
- 1701.02743 [astro-ph.GA]

pdfDOI

reference search19 citations

ZOMG – I. How the cosmic web inhibits halo growth and generates assembly bias

#8

(Oct 13, 2016)

Published in:
- Mon.Not.Roy.Astron.Soc. 469 (2017) 1, 594-611
•
e-Print:
- 1610.04231 [astro-ph.CO]

pdfDOI

reference search83 citations

Observational properties of simulated galaxies in overdense and average regions at redshifts z ≃ 6–12

#9

(Nov 10, 2014)

Published in:
- Mon.Not.Roy.Astron.Soc. 451 (2015) 1, 418-432
•
e-Print:
- 1411.2626 [astro-ph.GA]

pdfDOI

reference search15 citations

Simulating the H2 content of high-redshift galaxies

#10

(Mar 27, 2014)

Published in:
- Mon.Not.Roy.Astron.Soc. 446 (2015) 4, 3330-3345
•
e-Print:
- 1403.7132 [astro-ph.GA]

pdfDOI

reference search15 citations

Galaxy Formation in Heavily Overdense Regions at z~10: the Prevalence of Disks in Massive Halos

#11

(Jun, 2011)

Published in:
- Astrophys.J.Lett. 738 (2011) L19
•
e-Print:
- 1106.1214 [astro-ph.CO]

pdfDOI

reference search13 citations

The temperature of hot gas in galaxies and clusters: baryons dancing to the tune of dark matter

#12

et al.

(Dec, 2010)

Published in:
- Astrophys.J. 734 (2011) 62
•
e-Print:
- 1012.2870 [astro-ph.GA]

pdfDOI

reference search8 citations

The Dark Side of QSO Formation at High Redshifts

#13

(Oct, 2010)

Published in:
- Astrophys.J. 736 (2011) 66
•
e-Print:
- 1010.3715 [astro-ph.CO]

pdfDOI

reference search19 citations

Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models

#14

(Feb, 2010)

Published in:
- Astrophys.J. 716 (2010) 1095-1104
•
e-Print:
- 1002.4200 [astro-ph.CO]

pdfDOI

reference search26 citations

Dissecting Galaxy Formation: I. Comparison Between Pure Dark Matter and Baryonic Models

#15

Emilio Romano-Díaz
(
- Kentucky U.
)
,
Isaac Shlosman
(
- JILA, Boulder and
- NIST, Boulder
)
,
Clayton Heller
(
- Georgia Southern U.
)
,
Yehuda Hoffman
(
- Hebrew U.
)

(Jan, 2009)

Published in:
- Astrophys.J. 702 (2009) 1250-1267
•
e-Print:
- 0901.1317 [astro-ph.CO]

pdfDOI

reference search112 citations

Disk Evolution and Bar Triggering Driven by Interactions with Dark Matter Substructure

#16

(Sep, 2008)

Published in:
- Astrophys.J.Lett. 687 (2008) L13
•
e-Print:
- 0809.2785 [astro-ph]

pdfDOI

reference search42 citations

Erasing Dark Matter Cusps in Cosmological Galactic Halos with Baryons

#17

(Aug, 2008)

Published in:
- Astrophys.J.Lett. 685 (2008) L105
•
e-Print:
- 0808.0195 [astro-ph]

pdfDOI

reference search162 citations

DTFE analysis of the PSCz local Universe: Density Field and Cosmic Flow

#18

(Jul, 2007)

e-Print:
- 0707.2607 [astro-ph]

pdf

reference search2 citations

Evolution of Phase-Space Density in Dark Matter Halos

#19

Yehuda Hoffman
(
- Hebrew U.
)
,
Emilio Romano-Diaz
(
- Kentucky U.
)
,
Isaac Shlosman
(
- Kentucky U.
)
,
Clayton Heller
(
- Georgia Southern U.
)

(Jun, 2007)

Published in:
- Astrophys.J. 671 (2007) 1108
•
e-Print:
- 0706.0006 [astro-ph]

pdfDOI

reference search49 citations

Evolution of Characteristic Quantities for Dark Matter Halo Density Profiles

#20

Emilio Romano-Diaz
(
- Hebrew U. and
- Kentucky U.
)
,
Yehuda Hoffman
(
- Hebrew U.
)
,
Clayton Heller
(
- Georgia Southern U.
)
,
Andreas Faltenbacher
(
- UC, Santa Cruz
)
,
Daniel Jones
(
- Kentucky U.
)

et al.

(Oct, 2006)

Published in:
- Astrophys.J. 657 (2007) 56-70
•
e-Print:
- astro-ph/0610090 [astro-ph]

pdfDOI

reference search32 citations

Constrained simulations of dark matter halos

#21

Yehuda Hoffman
(
- Hebrew U.
)
,
Emilio Romano-Diaz
(
- Hebrew U.
)
,
Andreas Faltenbacher
(
- UC, Santa Cruz
)
,
Daniel Jones
(
- Kentucky U.
)
,
Clayton Heller
(
- Georgia Southern U.
)

et al.

(Oct, 2005)

Published in:
- EAS Publ.Ser. 20 (2006) 15
•
Contribution to:
- 21st IAP Colloquium on Mass Profiles and Shapes of Cosmological Structures
•
e-Print:
- astro-ph/0510439 [astro-ph]

pdfDOI

reference search0 citations

Constrained cosmological simulations of dark matter halos

#22

Emilio Romano-Diaz
(
- Hebrew U. and
- Kentucky U.
)
,
Andreas Faltenbacher
(
- UC, Santa Cruz
)
,
Daniel Jones
(
- Kentucky U. and
- Georgia Southern U.
)
,
Clayton Heller
(
- Georgia Southern U.
)
,
Yehuda Hoffman
(
- Hebrew U.
)

et al.

(Aug, 2005)

Published in:
- Astrophys.J.Lett. 637 (2006) L93-L96
•
e-Print:
- astro-ph/0508272 [astro-ph]

pdfDOI

reference search31 citations

Local supercluster dynamics: External tidal impact of the PSCz sample traced by optimized numerical least action method

#23

(Jun, 2005)

Published in:
- Astron.Astrophys. 440 (2005) 425
•
e-Print:
- astro-ph/0506372 [astro-ph]

pdfDOI

reference search4 citations

Emilio Romano-Diaz

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